Spectroscopy and asteroseismic modelling of the red giant binary system KIC 10841730
Stellar modelling is crucial for understanding the structure and age of stars. The accuracy of a stellar model is limited by the constraints from observations and the theory behind the physical processes. Gravitationally bound stars of a binary system provide an excellent opportunity for a combined study, which provides strong constraints on the
Schimak, Lea et al.
Fecha de publicación:
7
2024